Inflationary models with Ω ≠ 1

Details Inflationary models with Ω ≠ 1 Inflationary models with Ω ≠ 1

Nov 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991phlb..271...52e&link_type=abstract

Physics Letters B, Volume 271, Issue 1-2, p. 52-60.

Physics

27

Scientific paper

We describe the general features and a few specific models of inflationary cosmology that lead to Ω≠1 today, solve all standard problems of classical cosmology, and generate density perturbations that may be responsible for the formation of structures in the universe. Further development along these lines may require a more elaborate analysis of the initial conditions, both for the classical evolution and for the density perturbations.

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